The Hulse-Taylor Binary (PSR B1913+16,
PSR J1915+1606, or PSR 1913+16, aka the Hulse-Taylor Pulsar)
is a Binary Star system consisting of a Pulsar
and a second Neutron Star.
It was the first binary pulsar identified, in 1974,
and it is well know for the study of its orbital decay
that serves as evidence supporting the theory of General Relativity.
- Aquila - constellation.
- 19h13m12.4655s - Right Ascension.
- +16deg01m08.189s - Declination.
- 21000ly - distance.
- 1.441 - mass(solar).
- 59ms - rotation.
(pulsar,neutron star,binary star)
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